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0066-frame-C09  Page 43  Friday, January 18, 2002  11:01 AM









                         A 3-port I element can be used to represent the rotational kinetic energy for the case of rotation about
                       a fixed point (no translation). The constitutive relation is simply Eq. (9.25). The kinetic energy is then


                                                         T =  1
                                                              --ω h⋅
                                                              2
                            h
                       where   is the angular momentum with an inertia tensor defined about the fixed point. If the axes are
                       aligned with principal axes, then

                                                              --I y ω y +
                                                   T =  1 --I x ω x +  1  2  1 --I z ω z 2
                                                           2
                                                       2      2      2
                         The total kinetic energy for a rigid body that can translate and rotate, with angular momentum defined
                       with reference to the center of gravity, is given by

                                                     T =  1 --mV G +  1  ⋅
                                                              2
                                                                 --ω h G
                                                          2      2
                              2
                       where  V G =  V x +  V y +  V z .
                                           2
                                       2
                                   2
                       Rigid Body Dynamics
                       Given descriptions of inertial properties, translational and angular momentum, and kinetic energy of a
                       rigid body, it is possible to describe the dynamics of a rigid body using the equations of motion using
                       Newton’s laws. The classical Euler equations are presented in this section, and these are used to show
                       how a bond graph formulation can be used to integrate rigid body elements into a bond graph model.

                       Basic Equations of Motion
                                                                   p
                       The translational momentum of the body in Fig. 9.30 is   = m  , where m is the mass, and V   is the
                                                                        V
                       velocity of the mass center with three components of velocity relative to the inertial reference frame x o ,
                       y o , z o . In three-dimensional motion, the net force on the body is related to the rate of change of momentum
                       by Newton’s law, namely,
                                                              d
                                                           F   = ----- p
                                                              dt

                       which can be expressed as (using Eq. (9.9)),

                                                           ∂ p
                                                       F   = ------  +  Ω ×  p
                                                           ∂t
                                                             rel
                       with   now relative to the moving frame x a , y a , z a , and Ω   is the absolute angular velocity of the rotating
                           p
                       axes.
                         A similar expression can be written for rate of change of the angular momentum, which is related to
                       applied torques  T   by

                                                           ∂h
                                                       T   = ------  + Ω ×  h
                                                           ∂t
                                                             rel
                            h
                       where   is relative to the moving frame x a , y a , z a .

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